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California State University, Fresno
Department of Electrical and Computer Engineering
ECE 90L Principles of Electronic Circuits Laboratory
Experiment No. 1: Introduction to the Digital Storage Oscilloscope
Welcome to the Principles of Electronic Circuits Laboratory. You will find the following equipment on your lab bench:
· Tektronix TDS 210 or 1002 Two Channel Digital Real-Time Oscilloscope
· GW Instek GDM-8245 Digital Multi-Meter (DMM)
· GW Instek SFG-1013 DDS Function Generator
· Mastech DC Power Supply HY3005D-3 Function Generator
· Dual ± 12 V power supply with breadboard
Within the cabinets are: BNC cables, banana plug adapters, variable resistors, capacitors, and inductors, additional
power supplies, and other equipment that will be made available to you over the course of the semester as you perform
your experiments. Identify all of the equipment (listed above) on the lab bench before proceeding.
The first experiment is intended to be an introduction to some of the hardware available to you in the laboratory—
specifically the Tektronix TDS 210 or 1002 oscilloscope, the GW Instek GDM-8245 Digital Multi-Meter (DMM), and
the GW Instek SFG-1013 DDS Function Generator. An oscilloscope (scope) is an electronic instrument that displays
a voltage input as a function of time, and is typically used to display and measure repetitive waveforms or transient
signals. It is one of the important diagnostic tools that can be used by an Electrical or Computer Engineer. In the
process of learning about the functionality of an oscilloscope, you will also learn how to measure the voltage and
period/frequency of various signals.
The Tektronix TDS 210 Oscilloscope
Oscilloscopes are used by engineers and technicians to display voltage waveforms and signals as a function of time.
Older displays consist of a glass cathode ray tube (CRT), an electron gun, x- and y-deflection plates, and a phosphor
screen that emits light when struck with a focused electron beam. The spot of light can be moved by horizontally and
vertically deflecting the beam of electrons — if moved rapidly enough, the moving spot will have the appearance of
displaying an image on the screen. Horizontal deflection typically occurs from left to right at a constant speed called
the sweep rate, while vertical deflection occurs in response to the strength of the applied voltage, resulting in a plot
of the waveform. The horizontal sweep is generated by applying a triggered, sawtooth voltage waveform (created
internally) across the x-deflection plates. Although newer LCD screens on digital oscilloscopes do not use a CRT,
understanding the principles of older oscilloscopes is benefitial toward learning how the current generation of digital
scopes operate.
Figure 1 illustrates the “sawtooth” voltage waveform applied to the horizontal deflection points. At point A of the
cycle, the beam starts to sweep the screen, uniformly, from left to right. At point B, the beam passes through the center
of the screen and, at C, moves to the end of its trace on the right. The beam then quickly “jumps” back to the starting
point at A′ within a few nanoseconds, where a new cycle begins. Both the sweep rate and the vertical sensitivity can
be adjusted by using controls on the front panel of the oscilloscope, an example of which is shown in Figure 2.
Figure 1: The “sawtooth” shape of the sweeping voltage V(t). At point A of the cycle, the beam starts to sweep the
screen, uniformly, from left to right. At point B, the beam passes through the center of the screen and, at C, is at the
right end of the trace. The beam then quickly “jumps” back to the starting point at A′ within a few nanoseconds, where
a new cycle begins.
Display Controls
To begin, turn on the oscilloscope by pressing the POWER button on the top of the device. Because the Tektronix
210/1002 is a dual input oscilloscope, you can choose to display a voltage waveform from either 1 of 2 inputs (or both
simultaneously), which are marked CH1 and CH2, respectively, on the front panel. Repeatedly pressing the MENU
button for CH 1 will turn the scope trace for Channel 1 ON and OFF. Likewise, pressing the MENU button for CH
2 will turn the scope trace for Channel 2 ON and OFF. You have the option of displaying one of the scope traces at
a time, or both simultaneously if multiple signals need to be measured. Initially, we are only interested in looking
at the voltage on Channel 1, so press the appropriate MENU buttons to turn CH 1 ON and CH 2 OFF. Under the
TRIGGER MENU, make sure that the Auto option is selected (you can toggle between options under Mode using
the 2nd soft key button from the bottom, just to the right of the LCD). Also, make sure that the Edge option is selected,
you are using a Rising Slope, your Source input is CH1, and you are using DC Coupling. Next turn the SEC/DIV
knob to 250 µs, and make sure the VOLTS/DIV knob for CH 1 is turned all the way to the left.
After the scope warms up, you will see a horizontal line on the screen. If you cannot find the beam, use the VERTICAL POSITION knob to center the line at 0.00 divs (0.00 V). Because we are only looking at CH1, only the
left-hand knob for the VERTICAL POSITION will be useful. Rotating the knobs applies a constant (negative or
positive) voltage across the horizontal/vertical deflection plates, causing the beam to move horizontally/vertically on
the screen—depending on the applied voltage (how far you turn the knob). Experiment with the knobs for a bit to move
the trace to arbitrary locations on the display. Can the display be completely moved off the screen? What happened,
and why? Explain this in your lab notebook.
Once the trace has been centered, use the DISPLAY option to adjust the brightness of the trace using the Contrast
Increase and Contrast Decrease buttons. Repeat the process for CH 2 as necessary, but this time center the trace
toward the top of the screen. Once CH 2 has been adjusted, press the MATH MENU button and select the – Operation. Select CH1-CH2 and you will see a third trace displayed on the screen, which is the algebraic subtraction of
the two signals. This corresponds, physically, to the vector subtraction (or interference) of two parallel signals. You
can also select CH2-CH1 if you wish, or choose to add the two signals together by selecting + under Operation. By
adjusting the VERTICAL POSITION of either beam, you will see the vector addition or subtraction move as well.
Once finished, press the MATH MENU soft key button once more to turn off the Math Operation.
Next, press the CH 1 MENU button and be sure that the Coupling is set to Ground. Repeat for CH 2. Then adjust both
VERTICAL POSITION knobs so that the beams are exactly centered at 0.00 div (0.00 V). Then press the DISPLAY
button and change the Format option from YT to XY, which will turn your line into a dot (you will not be able to see
it unless you adjust one of the VERTICAL POSITION knobs. In this mode, the oscilloscope is capable of plotting
two-dimensional graphs representing a function y = f (x). The plot here is achieved by eliminating the variable time t
between the two functions f (x) and y(t), where x(t) is the CH 1 input signal and y(t) is the CH 2 input signal. The
physical meaning of this operation is the vector summation (or interference) of the two perpendicular signals. When
both signals are periodic, the resulting graph is known as a “Lissajoux” figure. Press the Format button once again to
return to the previous mode of operation YT.
Figure 2: The front panel of a Tektronix Oscilloscope Model 210. In this figure, the input signal is applied to Channel
1, whose sensitivity is set to 10.0 V/div. The time base is set to 250 µs/div, meaning that the beam will travel each
division in 250 µs, or the entire screen in 2.5 ms. The trace on the screen shows a continuous change of the input
voltage from −2.0 div×10 V/div= −20.0 V to +2.0 div×10 V/div= 20 V with a period over 4 div ×250 µs/div =
1.0 ms time interval.
Time Base Controls
The time base (SEC/DIV) is an important feature of these oscilloscopes, as it allows for the measurement of different
frequencies and time scales within an electrical circuit. Adjusting the time base adjusts how slowly/quickly the signal
sweeps across the screen. Since the sweep rate is constant, the distance (which is measured in screen divisions—and
more specifically, centimeters) traveled by the spot is a measure of the corresponding travel time. Experiment a bit
with the SEC/DIV knob, noting the different rates which the display can be swept. You should notice that for very
slow sweep rates, you can see the voltage versus time signal slowly sweep from left to right across the screen.
Whenever you turn on the scope, you should be able to quickly adjust all of the settings discussed so far (except,
perhaps when using XY mode) to center an oscilloscope trace on the display, and to adjust the INTENSITY (if necessary). The position knobs, temporarily grounding the inputs, and locating the traces for CH1 and CH2 allow the
reference level (0 V) of the display to be arbitrarily set, so become familiar with them. Once you are finished, set the
SEC/DIV knob to 500 µs, and turn OFF CH 2.
Sensitivity Controls
Vertical deflection of the electron beam is produced by applying an external, direct- or alternating-current (DC or AC)
signal to the input/s of the scope. The degree of vertical deflection is affected by both the magnitude of the input signal
as well as the sensitivity of the scope, which can be adjusted by using the VOLTS/DIV knob. Pressing the CH 1
MENU button, you can choose what kind of Coupling you wish to allow into the oscilloscope (Ground, DC, or AC.
When the Coupling button is pressed so that Ground is chosen, the input signal grounded—preventing any vertical
deflection of the beam. This position is typically useful for establishing a reference position somewhere on the display
and/or finding the beam. While the input is grounded, wherever the beam is moved to on the screen vertically (which
can be done arbitrarily using the VERTICAL POSITION knob) will determine the vertical location that corresponds
to 0 V, or ground. You should always know where ground is referenced to on the display for both CH1 and CH2 while
examining signals on the oscilloscope.
Unlike Ground, when the Coupling button is in the AC position, only the DC (constant) component of the signal will
be filtered from the input, which means that the AC (changing) component of the signal will still be displayed. And
finally, it is only when the button is in the DC position that the oscilloscope will display the actual waveform input into
the device—which includes both both the DC and AC components of the signal. The advantage of using AC coupling
over DC coupling occurs when you are trying to measure small variations of a signal that contain a large DC bias. As
an example, consider the relatively small “ripple” (5 mV) on the output of a typical DC power supply (say 5 V). With
DC coupling, increasing the input sensitivity in an attempt to see the small variation will send the trace off the top of
the screen. However, with AC coupling, the 5 V level will be suppressed and the sensitivity can be greatly increased
while retaining the trace on the center of the display.
Use the 5 V DC power supply to confirm this behavior (turn ON the power to the Mastech DC Power Supply
HY3005D-3). Use a BNC-banana adapter in conjunction with a BNC cable to hook up the +5 [email protected] voltage supply
on the Mastech Power Supply to the oscilloscope. Make sure the tab marked GND on the banana plug adapter is
plugged into the ground plug of the voltage supply. However, before you attach the output of the power supply to the
scope, first verify that you have a 5 V signal by connecting the output to the leads of the GW Instek Digital Multimeter
(DMM). Note that you must plug the leads for the DMM into the appropriate plugs (and have selected the DC voltage
button) to measure the voltage of the power supply. Once this has been done, using DC coupling on the oscilloscope,
re-verify that the output voltage of the power supply is correct. If you then try to examine the ripple more closely by
increasing the sensitivity (turning the VOLTS/DIV knob to the right), the trace will soon driven off the edge of the
display. With AC coupling, the DC level is suppressed and the ripple can be observed in detail; measure its amplitude
and compare it to the DC level. What happens if you gently wiggle the cable? Why?
Trigger Controls
The triggering circuitry is the means by which the oscilloscope is able to provide repeated “snapshots” of a repetitive
signal. By controlling the threshold voltage of triggering and slope polarity, the user is provided with great flexibility
in the appearance of the display and the utility of the scope for capturing elusive signals. Some further details of scope
operation are required to understand the concept of triggering.
As mentioned previously, the horizontal sweep of the electron beam is controlled by the timebase circuitry (the
SEC/DIV knob). The beam sweep is driven by the application of a ramp voltage to the horizontal deflection plates,
which serves to move the beam across the face a distance proportional to the elapsed time from a trigger event. The
occurrence of the trigger event marks the start of the linear ramp. By slowing the timebase to about 1 s/div, the actual
deflection of the beam can be slowed to the point where the resulting luminous waveform can be observed crossing
the display from left to right.
To examine the effects of the trigger settings on the triggering of the display, use the output available on the SFG-1013
function generator to generate a 600 Hz triangle wave (use the WAVE button) as the input signal for CH 1. Hook up
the input to CH 1 on the scope and increase the sensitivity to 5 V/div. Adjust the amplitude on the function generator
so that the amplitude of your triangle wave is exactly 5 V (peak to peak), and select a 500 µs/div sweep speed on the
oscilloscope. With the trigger Source set for CH1 (note there are 5 options—CH1 for Channel 1, CH2 for Channel
2, and Ext for an external trigger, Ext/5 which divides the external trigger by 5, and AC Line which expects an AC
signal), the TRIGGER LEVEL knob rotated to be just above 0 V, and the Slope option set to detect on the rising
edge of a pulse, a stable trace showing the triangle wave should appear. Adjust the horizontal position of the trace until
its starting position is seen on the display. Next, adjust the TRIGGER LEVEL by adjusting the knob to the left and
right. Notice that as the threshold for the trigger is increased (moving the trigger toward the right), the starting point
of the trace changes (in this case toward the left). Likewise, adjusting the threshold for the trigger toward a negative
voltage (moving the trigger increasingly toward the left), the starting point of the trace moves in the opposite direction.
Refer to Figure 3 for a pictorial representation of the various triggering combinations. Switch the trigger SLOPE and
observe the changes to the displayed waveform. The SLOPE selector chooses whether the trigger event will occur
when moving through the threshold from a high voltage to a low voltage (falling edge/negative slope) or from a low
to high voltage (rising edge/positive slope). Refer again to Figure 3.
Finally, setting the trigger level too low or too high (outside the bounds of the signal amplitude) results in loss of
triggering and an unstable “running” waveform. You can observe this if you decrease the input amplitude of the signal
Figure 3: Effects of slope and the threshold on triggering.
by using the AMPLITUDE knob on the function generator. Decreasing the TRIGGER LEVEL down toward the
voltage level of waveform will restore a stable trace. Notice also what happens if you switch the trigger Source to
CH2. Explain your results for both cases.
Next, examine of the effects of the external trigger selection EXT. It is with this setting that an additional, betterconditioned signal can be used to trigger the scope while observing a relatively weak signal—one that is too weak
when using internal triggering, as discussed above. For example, you may again observe the ripple on the DC power
supply or the stray signal picked up by a loose lead, using the 600 Hz, AC signal to trigger the scope externally. External triggering is accomplished by connecting the signal to be used for triggering to the external trigger input EXT
TRIG of the scope and selecting Ext on the trigger Source button.
When you are finished, display a 600 Hz, 5 V peak-to-peak sinewave using CH 1 on the scope. Make whatever adjustments are necessary to display a stable waveform. Then start from 500 µs/div and increase the timebase to larger
settings (slower sweeps), which is simply a longer “snapshot” of the signal being displayed, but with less detail. Remember that the 600 Hz signal has not changed; the beam sweeps more slowly, so only more transitions are displayed.
Moving to much smaller timebase settings (faster sweeps), more detail can be seen at the expense of the “big picture”.
However, notice the decrease in intensity of the trace as the electron beam moves more swiftly over the screen at faster
time base settings. Finally, adjust the frequency of the sinewave from 6 Hz all the way to 6 MHz by powers of 10 and
adjust the time base setting as necessary to continue to provide a “clean” display. Comment on your results.
Returning to a timebase around 500 µs/div and a frequency of 600 Hz, confirm with the oscilloscope that the period of
the 5 V AC signal is 600 Hz. Adjust the trigger level if necessary to achieve a stable display. Measure the horizontal
distance between the two closest points where the waveform crosses the baseline (0 V level) with the same slope.
(Note that there are two zero crossings per cycle, each with different slope.) Multiply this number of divisions by the
timebase setting (time/div); the resulting time T is known as the period.
How short a time can be read by this oscilloscope? This can be estimated by the smallest timebase setting. In practice,
this setting may result in a trace too weak to be seen—thus the so-called writing speed of the oscilloscope may also
limit the shortest time that can be accurately determined, as will the bandwidth of the input amplifiers.
Dual Trace Operation
The availability of two independent input channels greatly facilitates comparison of two signals. To do this, turn on
both Channels. While displaying the 5 V, 600 Hz sinusoidal signal on CH 1, using it as a trigger source, observe
the signal from a loose BNC cable on CH 2. You will probably observe “spikes” and other types of electrical noise,
depending on the sensitivity level. You should attempt to explain why this noise is “locked” to the signal on CH 1. For
a more dramatic effect, touch your finger to the CH 2 input conductor from the BNC cable. The noise probably has
much higher amplitude and is still locked to the calibration signal. Finally, while holding the bare lead in one hand,
touch the metal frame of the table and observe the noise signal on CH 2. Attempt to explain your observations.
Next, apply the 0 - 20 V input from the Mastech power supply to CH 2 on the oscilloscope using the red and black
banana plugs, making sure that the plug with the GND tab is attached to the common, black output from the power
supply. While displaying both Channels on on the oscilloscope, adjust the Coupling control to DC for both channels,
and observe your results when using the MATH MENU options. As you do so, adjust the amplitude of the DC signal
using the + VOLTS knob on the dual power supply. What happens, and why? Finally, try various combinations of
AC, GND, and DC, and observe your results. When the knobs are in the AC position and you vary the amplitude of
the DC voltage from the dual power supply, what happens? Why?
X-Y Mode
Once you are comfortable with the dual trace operation of the oscilloscope, set the amplitude of the DC signal into CH
2 to 5 V and select XY operation of the scope using the Format option after hitting the DISPLAY button. Now, the
voltages into CH 1 and CH 2 are functions of each other. Can you justify which channel is a function of the second
channel, based upon what you see on the screen? Next, switch the inputs, so that the sinusoid is input into CH 2 and
the DC voltage into CH 1. What changed, and why?
Additional Display Options
Next press the MEASURE button and note that there are various measurements about the waveforms that can be
displayed for both Channels 1 and 2. Experiment with the various measurement options and explain as many as you
can in your laboratory notebook. Next press the CURSOR button and choose Time under the Type option. You can
then move the two VERTICAL POSITION knobs to give you a measurement of the time difference between the two
vertical lines. This can be used to help you make measurements in time. Similarly, if you choose Voltage under the
Type option, you can make similar measurements with respect to voltage. Once finished, turn the CURSOR Type to
Finally, press the ACQUIRE button and note that you can continually sample the voltage versus time plot by selecting
Sample, choose to display the peak voltages by selecting Peak detect, or display an average of a number of voltages
by selecting Average and then adjusting the Averages button. Explain the difference between the waveforms for each
case, and describe what the oscilloscope is doing.
Provide a brief conclusion based upon what you have learned today and both partners will turn in the lab book at the
beginning of the next laboratory session. No group report is necessary for this laboratory.
In addition to my own work, several people have allowed me to adapt portions of their lab manuals into this laboratory
procedure. I would like to gratefully acknowledge the following people for giving me permission to use their materials:
Dr. Larry Owens, Professor, Electrical and Computer Engineering Department, California State University, Fresno.
Dr. George Watson, Associate Dean, College of Arts & Sciences, University of Delaware.
Dr. Jeffrey Urbach, Associate Professor and Chair, Department of Physics, Georgetown University.